The RS-II model is a based on a modification of the RS-I Braneworld cosmology model[1]}, where the hierarchy problem is solved by embedding two 3-branes in a five-dimensional bulk where one of the branes contains the Standard Model particles. The RS-II braneworld cosmology removes one of the 3-branes and recovers both Newtonian gravity and General Relativity as its limiting cases[2]}. Since another braneworld cosmology scenario in the form of Dvali-Gabadadze-Porrati (DGP) model [3]}, [4]} can produce some effects on the late-time evolution of the universe, it becomes very interesting to see if one can address late-time acceleration issues using the RS-II model as well. In this direction, there have been several works in recent times which have addressed Quintessence in the RS-II Braneworld scenario[5]}, [6]}, [7]}. We can write the total action of the RS-II Model inclusive of both the scalar and the background fluid term as
\(S = S_{RS} + S_{B} + S_{\phi } = \\ \int d^5 x \sqrt{-g^{(5)}} \left( \Lambda ^{(5)} + 2 R^{(5)} \right) + \int d^4 x \sqrt{-g} \left(\lambda -\frac{1}{2} \mu (\phi ) (\nabla \phi )^2 - V(\phi ) + \mathcal {L}_{B} \right)\) 
